Chemical Composition of RM_1-390 - Large Magellanic Cloud Red Supergiant
A high resolution spectroscopic observation of the red supergiant star RM_1-390 in the Large Magellanic Cloud was made from a 3.6 m telescope at the European Southern Observatory. Spectral resolving power was R=20,000, with a signal-to-noise ratio S/N > 100. We found the atmospheric parameters of...
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| Asıl Yazarlar: | , , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
The Korean Space Science Society
2017-09-01
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| Seri Bilgileri: | Journal of Astronomy and Space Sciences |
| Konular: | |
| Online Erişim: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2017/v34n3/OJOOBS_2017_v34n3_199.pdf |
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